New Hα instrumentation at the Kanzelhöhe Solar Observatory

Details New Hα instrumentation at the Kanzelhöhe Solar Observatory New Hα instrumentation at the Kanzelhöhe Solar Observatory

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..729h&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

Sun, Instrumentation, Hα, Waves

Scientific paper

We present a short overview over new instrumentation developed at the Kanzelhöhe Solar Observatory. The main advantages of this observatory is a permanent staff which permits continuous solar monitoring. Due to the high quality of data (especially Hα) and the incorporation of the observatory into several international solar observing campaigns new developments are done continuously. Observing in the wings of Hα provides the possibility to study different phenomena such as waves and oscillation propagation.

Affiliated with

Also associated with

No associations

Rating

New Hα instrumentation at the Kanzelhöhe Solar Observatory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New Hα instrumentation at the Kanzelhöhe Solar Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Hα instrumentation at the Kanzelhöhe Solar Observatory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1153002